modelo n merico para la generación de mapas de radiación solar.

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# &
Go = Io /0
= 1 + 0,03344 cos(j − 0,048869) j ( j =
2πj
365,25
/+0
j *
# 4=? $ Boc (W/m2) Boc = Go exp{−0,8662TLK mδR (m)}
/40
$ %
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m /A B CDC0
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m = (p/po )/ sin href
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o + 6,07995) 1,636
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# m #
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/D0
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δR (m) = 1/(10,4 + 0,718)
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ho # Ao ( #
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/+0
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/40
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/?0
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=
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sin δexp
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/+60
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A∗LN = Ao − AN
−pi ≤ A∗LN ≤ pi ALN = A∗LN
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A∗LN < −pi ALN = A∗LN + 2pi
)
! δexp < 0 ho ≥ 0
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# Dic = Dhc F (γN )
F (γN )
F (γN ) = ri (γN ) + (sin γN − γN cos γN − π sin2 (γN /2))N
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ri(γN ) ! "
ri (γN ) = (1 + cos γN )/2
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N N = 0,00263 − 0,712Kb − 0,6883Kb2
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Ri = ρg Ghc rg (γN )
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